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Within both methods the OTOC is given as a sum of two contributions, corresponding to left and right moving modes. The contributions have different Lyapunov exponents, $\\lambda_L^{\\pm}=\\frac{2\\pi}{\\beta}\\frac{1}{1\\mp \\ell \\Omega}$, where $\\Omega$ is the angular velocity and $\\ell$ is the AdS radius. Since $\\lambda_L^{-} \\leq \\frac{2\\pi}{\\beta} \\leq \\lambda_L^{+}$, there is an apparent co"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1903.09086","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-03-21T16:15:39Z","cross_cats_sorted":[],"title_canon_sha256":"642c8b63e384ec30aaced79c01103fbdbead6bc941835601b2d60015cc2f8982","abstract_canon_sha256":"3b3ccf08e940adf13f2d1f791f182242765f11b532d750ee5bee9bdaa63063ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:44:21.442945Z","signature_b64":"PduZ8zi2pYOpMq5f4XkU3nJtAdktH7POJFZBR9UX4+yeEaYZM1XwQ72THoAfRNsFMsESM1eKt2H9mrb7SB9NAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5baeab482345f53eccd005ad7f27cad2181d096fe05632557ff67d2700e48260","last_reissued_at":"2026-05-17T23:44:21.442303Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:44:21.442303Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Chaos Bound in Rotating Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Junggi Yoon, Keun-Young Kim, Viktor Jahnke","submitted_at":"2019-03-21T16:15:39Z","abstract_excerpt":"We study out-of-time-order correlators (OTOCs) of rotating BTZ black holes using two different approaches: the elastic eikonal gravity approximation, and the Chern-Simons formulations of 3-dimensional gravity. 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